X-ray Beamline Design 2012cheiron2012.spring8.or.jp/text/Lec5_S.Goto.pdf · G x y z π π π π π...

62
1 X-ray Beamline Design 1 X-ray Monochromator Shunji Goto SPring-8/JASRI September 25, 2012 Cheiron School 2012

Transcript of X-ray Beamline Design 2012cheiron2012.spring8.or.jp/text/Lec5_S.Goto.pdf · G x y z π π π π π...

  • 1

    X-ray Beamline Design 1

    X-ray Monochromator

    Shunji GotoSPring-8/JASRI

    September 25, 2012

    Cheiron School 2012

  • 2

    Outline

    1. Introduction2. Light source3. X-ray Monochromator

    Fundamental of Bragg reflectionDynamical theoryDuMond diagram ~ extraction of x-rays from SRDouble crystal monochromatorCrystal cooling

    4. Example of beamlines at SPring-85. Summary

  • 33

    SR

    Experimental station

    Exp. hallRing tunnel

    Front-end

    Beamline structureBeamline = “Bridge” between light source & experimental station

    Transport and processing of photonsphoton energy, energy resolution,beam size, beam divergence, polarization,..

    Light source

    Monochromator, mirror

    shutter, slit

    pump,..

    Vacuumprotection of ring vacuum and beamline vacuum

    Radiation safety

    Shielding and interlock

    Bending magnet

    Insertion device

    Shielding hutch

    Optics & transport

  • 4

    Light sources & X-ray optics

    - White or monochromatic

    - Energy range

    - Energy resolution

    - Flux & flux density

    - Beam size at sample (micro beam?,...)

    - Beam divergence/convergence at sample (Resolution in k-space)

    - Higher order elimination w/ mirror

    - Polarization conversion

    - Spatial coherency

    ....

    Check points to be considered for your SR application:

    Light source, monochromator, mirror,

    and other optical devices and components

  • 5

    BL classification (energy region)

    Photon energy (eV)

    IR

    101 103 104 105

    Undulator

    Bending magnet

    Wiggler

    SX-PES

    102

    Earth,..HP/HT

    Inelastic

    Inelastic

    SAXS

    PX

    XAFSPowder XRD

    HP/HT XRD

    NRS

    SAXS

    SX-MCD

    PEEM

    HX-PES

    HXSXIR

    100

    Visible ~ UV~

  • 6

    BL classification (energy resolution)

    Undulator

    Bending magnet

    White

    Earth,..HP/HT

    10-7 10-5 10-3

    XAFSSAXS

    XAFS

    SAXS

    PX

    PX

    Inelastic

    NRSHX-PES

    Topograph

    Topograph

    Surface ・interface XRF

    Powder XRD

    Wiggler Inelastic

    Microbeam, imagingXMCD

    Imaging

    HP/HT XRD

    Single crystal XRD

    Energy resolution (ΔE/E)

  • 7

    Light sources (1)

    Bending magnet or insertion devices ?

    Bending magnet:for wide energy range, continuous spectrum

    for wide beam application for large samples

    Undulator (major part of 3GLS beamline):for high-brilliance beam

    for micro-/ nano-focusing beam

    Wiggler:for higher energy X-rays > 100 keV. 1012

    1014

    1016

    1018

    1020

    1022

    Bril

    lianc

    e (p

    h/s/

    mm

    2/m

    rad2

    /0.1

    % B

    .W.)

    100 101 102 103 104 105 106

    Photon energy (eV)

    Brilliance for SPring-8 casePower, brilliance, flux density, partial flux,.. can be calculated using code.

    e.g. “SPECTRA” by T. Tanaka & H. Kitamura

  • 8

    Light sources (2)Angular divergence and band width

    Core part we need

    Bending magnet

    Undulatorc

    r λλ

    γσ 1597.0≈′

    nNK

    N un

    r21

    21

    2

    2+=≈′ γλ

    λσ

    nNEE 1

    ≈Δ

    SPring-8 in-vacuum undulator

  • 9

    γψ 1≈vPower distribution

    consth ≈ψ

    γψ 1≈vγψ Kh ≈

    K: deflection parameter (K= 0.5~2.5)

    ]A[]rad[]m[]T[]GeV[27.1]kW[ 22tot IRBEP φ= ]A[]m[]T[21]GeV[27.1]kW[ 20

    2tot ILBEP =

    Total power

    E= 8 GeV, I= 0.1 A, B= 0.68 T, R= 39.3 m Ptot= 0.15 kW/mrad

    B0= 0.87 T, L= 4.5 mPtot= 14 kW

    ]m[ArcL ( )uzB λπ2sin220

    Light sources (3)

    Bending magnet Undulator

    Kilowatt of SR power mostly eliminated before/by monochromator

  • 10

    X-ray MonochromatorX-ray monochromator is key component for SR experiments:

    length gauge for structure analysis,energy gauge for spectroscopy,...

    Principle of x-ray monochromator

    Photon energy tuning Bragg’s law

    Energy resolution source divergence, Darwin width,..

    Flux (throughput) related to Darwin width

    Understanding the dynamical theory for large & perfect crystal

    Practical of the monochromator

    Double-crystal monochromator for fixed-exit

    Single-bounce monochromator is for limited case

    Crystal cooling

    High heat load depending on light source

    Mechanical engineering issues

  • 11

    λθ md =Bsin2

    θ θ d

    dsinθ dsinθ

    hKKQ =−= 0s

    Bragg’s law in real space Laue condition (Kinematical)in reciprocal space

    Reciprocal lattice vector h- Normal to net plane- Length = 1/d

    1) Phase matching on the single net plane by mirror-reflection condition.

    2) Phase matching between net planes.

    net plane (spacing d)

    Reciprocal lattice vector h

    Scattering vector Q

    Scattered wave Ks

    Incident wave K0 θ θ

    Bragg reflection

  • 12

    Ewald sphere

    Ewald sphere:

    When a reciprocal lattice point is on the Ewald sphere, Bragg reflection occurs.

    Reciprocallattice points

    0K

    SK01 KRadius == λ

    h

  • 13

    Top view

    Side view

    [100]

    [011]

    [010]

    [001]

    (400)

    (511)

    (111) : 3.1356 Ǻ(311) : 1.6375 Ǻ

    (400) : 1.3578 Ǻ

    (511) : 1.0452 Ǻ

    a

    a

    d-spacing

    (111) (311)

    222 lkh

    ad++

    =

    Miller indices and d-spacing for silicon

    a = 5.431Å

    Diamond : a = 3.567Å

  • 14

    ( ) ( ) ( )∑ ⋅=j

    jj iEfF rhhh π2exp,

    ( ) ( ) ( ){ }∑ ++=j

    jjjj lzkyhxiEfF π2exp,hh

    lkh ,, Mixture of odd and even numbers0=F

    All odd, or, all even numbers, and m: integer,

    mlkh 4=++ fF 8= 8 atoms in phase

    14 ±=++ mlkh ( ) fiF ±= 14

    24 ±=++ mlkh 0=F

    Half contribute with phase shift ±π /2

    lkh ,,

    Half cancel with π

    For diamond structure

    Structure facrtor Sum of atomic scattering with phase shift in the unit cell

    Position of atoms in the unit cell for diamond structure

    (xj, yj, zj) =

    (0, 0, 0)1, (1/4, 1/4, 1/4)2,

    (1/2, 1/2, 0)3, (3/4, 3/4, 1/4)4,

    (0, 1/2, 1/2)5, (1/4, 3/4, 3/4)6,

    (1/2, 0, 1/2)7, (3/4, 1/4, 3/4)8

    1

    2zy

    x

    34

    5

    6

    7 8Atomic scattering factor

    Crystal structure factor for diamond structure

  • 15

    (400), (220),...

    All in phase

    [100]

    [011]

    (400)

    (511)

    a

    (111) (311)

    (111), (311),... Half contribute with phase shift ±π /2

    (200)

    (011), (200),...

    Half cancel with π

    Forbidden reflection

    (011)

    ( ) fiF ±= 14fF 8=

    0=F

    Crystal structure factor for diamond structure

  • 1616

    X-ray monochromator using perfect crystal

    Perfect single crystal: silicon, diamond,..

    0

    20

    40

    60

    80

    100

    120

    0 5 10 15 20 25 30Bragg angle (deg)

    Pho

    ton

    ener

    gy (k

    eV)

    Si 111 refl.

    Si 311 refl.

    Si 511 refl.

    e.g. for SPring-8 standard DCM

    Bragg angle: 3~27°

    Photon energy tuning:

    Crystal & lattice plane

    Bragg angle range

    Bsin][23984.12]keV[

    θÅhkldE =

  • 17

    ( ) ( ) 22 QQ GFII e ⋅=

    Peak intensity 2xN

    FWHM xx NNh 1~8858.0≈Δ

    Crystal size becomes larger narrower & higher, approaching delta function

    ( ) ( )( )( )

    ( )( )

    ( )llN

    kkN

    hhNG zyx

    ππ

    ππ

    ππ

    2

    2

    2

    2

    2

    22

    sinsin

    sinsin

    sinsin

    ⋅⋅=QLaue function:

    h, k, l: integer Intense peaks(hkl) reflection

    3-dim. Periodic structure

    0

    20

    40

    60

    80

    100

    -1.5 -1 -0.5 0 0.5 1 1.5 2 2.5

    120

    ( )( )h

    hNxπ

    π2

    2

    sinsin

    h

    One-dim. Laue function, Nx= 10

    Kinematical X-ray diffraction

    NxNy

    Nz

    cba zyx nnn ++

    Unit cell

    3-dimensional periodic structure of unit cell with number Nx, Ny, NzTotal scattering intensity becomes:

  • 18

    Dynamical theoryTwo-wave approximation

  • 19

    Kinematical to dynamical theory

    “Large & perfect” single crystal:1) Multiple scattering w/ h & -h reflection2) Extinction

    (Diffraction by “finite” number of net planes)

    Kinematical diffraction is invalid Dynamical theory must be applied.

    Net plane

    Incident wave Diffracted wave

    Extinction

  • 20

    Fundamental equation

    h, g,... : Reciprocal lattice points

    Eh, Eg : Fourier components of electric field

    K0 : Incident wave vector in vacuum

    kh : Wave vectors in the crystal

    χh : Fourier components of the polarizability (Negative values, 10-6~10-5)

    P= (eh・eg) : Polarization factor between h and g waves

    kh= k0 + h : Momentum conservation

    Fundamental equation is derived

    using Maxwell’s equations and introducing Bloch wave

    for 3-dimensional periodic medium (= perfect single crystal):

    ( )∑ ⋅=− −g

    gghghhh EE

    KKk eeχ2

    0

    20

    2

  • 21

    Two-wave approximation

    : Fourier components of the polarizability

    (Negative values, 10-6~10-5)

    : Polarization factor ( )

    Fundamental equation is reduced to the equation for

    two waves of incidence and “one” intense diffraction

    ( )∑ ⋅=− −g

    gghghhh EE

    KKk eeχ2

    0

    20

    2 ( ) hhEPEEKKk

    −+=− χχ 0002

    0

    20

    20A

    ( ) hhhh EEPEKKk

    002

    22

    B χχ +=−

    hh −χχχ ,,0

    ( )hP ee ⋅= 0 BPP θπσ 2cos:,1: ==

  • 22

    Two-wave approximation

    ( ) hhEPEEKKk

    −+=− χχ 0002

    0

    20

    20A

    ( ) hhhh EEPEKKk

    002

    22

    B χχ +=−

    hE0χ

    00Eχ

    0Ehχ

    Scheme of self-consistent wave field

    hhE−χ0E⇒

    hE⇒0E

    hE

    ( )( ) 40222220 KPkk hhh −=−− χχkk( ) 2002 1 Kk χ+=

    Using two equations, we obtain following secular equation:

    h

    h−

    Secular equation

    k : Mean wave number in the crystal

  • 23

    Boundary condition of wave vector

    Tangential component of wave vector must be continuous.

    Incident wave in vacuum

    Refracted wave in the crystal

    Bragg reflection in the crystal

    Reflected wave in the crystal

    Reflected wave in vacuum

    K0 Kh

    k0 kh

    Vacuum Crystal

    We must consider connections of waves from vacuum into the crystal and from the crystal to vacuum, to solve the equations.

  • 24

    Laue case and Bragg case

    K0 Kh

    n

    K0 Kh

    n

    Laue case(Transmission geometry)

    Bragg case(Reflection geometry)

  • 25

    Asymmetry ratio

    h

    bγγ 0=

    nK ⋅= 00 ˆγ

    nKhh ⋅= ˆγ

    Laue case: b>0

    Symmetric Laue case: b= 1

    Bragg case: b< 0

    Symmetric Bragg case: b= -1

    K0 Kh

    n

    n: normal vector to the surface

  • 26

    Dispersion surface( )( ) 40222220 KPkk hhh −=−− χχkk

    Two dispersion surfaces show the gap near Bragg condition.

    h

    kh

    k0 O

    H

    Reciprocal spaceReal space

    Secular equation is quartic equation, and it gives four-point solution on the n-vector,producing the dispersion surfaces.

    n-Laue

    n-Bragg

    K0 Kh

    n

    K0 Kh

    n

    Laue case

    Bragg case

    0K

    0K

    Laue case

    Bragg case

    kh= k0 + h

  • 27

    Deviation from Bragg condition

    Excitation errorGeometrical deviation ζ0 from Bragg condition:

    Distance between Ewald sphere and the reciprocal lattice point.

    ζ0 is positive when H is inside the Ewald sphere (by S. Miyake).

    O

    H

    0K

    SK 0ζ

    h

    ( )0

    20

    0 22

    Kh+⋅

    −≈hKς

  • 28

    Normalized deviation parameter W

    For symmetric Bragg case, sigma polarization:

    Parameter W is related to the gap between two dispersion surfaces

    and total reflection occurs at –1

  • 29

    Sign of deviation parameter W

    Angle deviation at fixed energy

    direction change of wave vector

    Energy deviation at fixed angle

    length change of wave vector

    h h0W

    00 →> WEE

    0K0K

    0EE =

  • 30

    Movement of tie point

    (3) Higher angleW> 1

    h

    kh

    k0 O

    H

    K0 Kh

    Vacuum

    Crystal

    h

    kh

    k0 O

    H

    K0 Kh

    Total reflection

    (1) Lower angleW< -1

    (2) Near Bragg condition-1< W< 1

    h

    kh

    k0 O

    H

    K0 Kh

    Dominant branch for thick Bragg-case crystal is close to O-sphere.

    Tie point moves by changing the incident angle

    at fixed photon energy (wavelength).

  • 31

    Calculation of polarizability

    hihrh χχχ +=

    For diamond structure

    ( ) Mc

    ehr effv

    r −′+−= 02

    λχ

    M

    c

    ehi efv

    r −′′−= 82

    πλχ

    ( )fZv

    r

    c

    er ′+−= 8

    2

    0 πλχ

    fv

    r

    c

    ei ′′−= 8

    2

    0 πλχ

    mlkh 4=++

    14 ±=++ mlkh

    0=== lkh

    ( )( ) Mc

    ehr effiv

    r −′++−= 02

    14π

    λχ

    ( ) Mc

    ehi efiv

    r −′′+−= 142

    πλχ

    χh: Fourier component of polarizabilityproportional to the structure factor

    vc: unit cell volume

    ( )EFv

    r

    c

    eh ,

    2

    λχ −=

    ( ) ( )Effhr ′+⇔ h0χ

    Atomic form factor + real part of anomalous factor

    ( )Efhi ′′⇔χImaginary part of anomalous factor

  • 32

    Amplitude ratio

    From the solution of the fundamental equations, we obtain the ratio r = Eh/E0 ( reflection coefficient)as a function of parameter W.

    For Bragg case, no absorption, and thick crystal:

    ( ) )1(1200

    −−−−==−

    WWWPP

    EEr

    h

    hr

    h

    h

    χχ

    γγ

    Total reflection

  • 33

    ( ) )1(1 22 −−−= WWWR

    hEEW

    χχθθθ 1sin22sin 0B

    2B ⎟

    ⎠⎞

    ⎜⎝⎛ +

    Δ+Δ=

    W: deviation parameter for s-polarization, symmetrical Bragg case

    Angular deviation

    Energy deviation

    Geometry for symmetrical Bragg case

    net plane

    K0

    Bθ SurfaceBθ

    Khθθ Δ+Bθθ Δ+B

    Refraction

    Total reflection region

    Darwin curve (intrinsic reflection curve for monochromatic plane wave)for Bragg case, no absorption, and thick crystal:

    Reflectivity (Darwin curve)

  • 34

    Darwin curve

    For Bragg case, no absorption, and thick crystal:

    0

    0.2

    0.4

    0.6

    0.8

    1

    1.2

    -5 -4 -3 -2 -1 0 1 2 3 4 5

    W

    Ref

    lect

    ivity

  • 35

    Reflectivity with absorption

    - symmetrical Bragg case, - s-polarization, - thick crystal

    12 −−= LLR

    ( ) ( )2

    2222222

    1

    41

    κ

    κκ

    +⎭⎬⎫

    ⎩⎨⎧ −++−−++

    =gWgWgW

    L

    rh

    hi

    rh

    igχχ

    κχχ

    == ,0hr

    rEEW

    χχθθθ 1sin22sin 0B

    2B ⎟

    ⎠⎞

    ⎜⎝⎛ +

    Δ+Δ=

    Reflectivity

    Note: No absorption curveDarwinRg →⇒== 0,0 κ

  • 36

    Reflectivity curve for silicon

    ・Width of 0.1~100 µrad・Peak ~1 with small absorption

    回折幅

    0

    0.2

    0.4

    0.6

    0.8

    1

    -100 -50 0 50 100Δθ (µrad)

    Ref

    lect

    ivity

    Si 111 refl. 10 keV

    Si 333 refl. 30 keV

    Examples for symmetrical Bragg case, with absorption, s-polarization and thick crystal:

    Si 111 refl., 10 keV

    ( )( )i

    i

    i

    r

    i

    r

    +×−=

    +×−=

    ×−=

    ×−=

    11030.7

    11066.3

    1048.1

    1078.9

    8_111

    6_111

    70

    60

    χ

    χ

    χ

    χ

    ( )( )i

    i

    i

    r

    i

    r

    +×−=

    +×−=

    ×−=

    ×−=

    11087.7

    11024.2

    1075.1

    1007.1

    10_333

    7_333

    90

    60

    χ

    χ

    χ

    χ

    Si 333 refl., 30 keV

  • 37

    Effective band width

    2Darwin

    2Bcot θθ Δ+Ω=

    ΔEE

    Energy resolution

    B2sin θ

    χhrEE

    ≈Δ

    Angular width(Darwin width)

    ( )hFhr ∝=ΔB

    Darwin 2sin2

    θχ

    θ

    Gaussian approximation for both light source and reflection curve

    EEΔRelative energy

    1−=W 1=W

    Incident angleBθ θ

    Darwin width

    Shift by refraction

    Kinematical Bragg condition

    Bcotθ−Slope:

    EEΔRelative energy

    Incident angle θ

    Energy resolution

    Effective band width

    Light source divergence φ

    Light source

    ΔW= 2

    The diagram helps to understand how we can extract x-rays from SR source.

    DuMond (angle-energy) diagram

  • 38

    Source divergence and diffraction width

    Divergence of undulator radiation ~ diffraction width

    - Bending magnet

    μrad60≈′rσ

    - Undulator (N= 140)μrad5r ≈′σ

    For SPring-8 case:

    - Undulatorωλ

    λγ

    σh

    11597.0 ∝≈′c

    r

    - Bending magnet

    Natural divergence

    ωλλσ

    h

    12

    ∝≈′u

    r N

    103

    0 20 40 60 80 100

    Photon energy (keV)

    FWH

    M (µ

    rad)

    102

    101

    100

    10-1

    Bending magnet

    Undulator

    Si 111 refl.

    Si 311 refl.

    Si 511 refl.

  • 39

    Energy resolution

    For usual beamline : ΔE/E=10-5~10-3

    22Bcot ωθ +Ω=

    ΔEE Ω: source divergence,

    ω: diffraction width

    Angle-energy diagram(DuMond diagram)

    φ

    Pho

    ton

    ener

    gy

    Light source distribution

    Δθ, φ

    Acceptance by crystal

    Resolution

    10-5

    10-4

    10-3

    10-2

    0 20 40 60 80 100Photon energy (keV)

    ΔE/E

    BM & Si 111 refl.

    BM & Si 311 refl.

    BM & Si 511 refl.

    Undulator & Si 111 refl.

  • 40

    DuMond diagram: undulator & DCMSPring-8 standard undulator

    (λu= 32 mm, N= 140, K= 1.34, E1st= 10 keV)

    + DCM (Si 111 refl.)

    10 keV (1st) 30 keV (3rd) 50 keV (5th)

    Wider slit increases unused photons (power) on the monochromator !

    Intensity distribution of

    undulator

    200

    ΔE(e

    V)

    -50 500φ (μrad)

    -200

    0

    600

    ΔE(e

    V)

    -50 500φ (μrad)

    -600

    0

    1000

    ΔE(e

    V)

    -50 500φ (μrad)

    -1000

    0

    φ

    Acceptance by crystal

    DE/

    E= 2

    x10-

    4

    50 μrad Undulator radiation: ( )2220 21 φγ++= KEE

  • 41

    DuMond diagram: undulator & DCM

    SPring-8 standard undulator + 20 μrad slit + Si 111 DCM10-keV photons 1.3x10-4

    100 μrad

    ΔE/E

    = 5x

    10-4

    -3

    -2

    -1

    0

    1

    2

    3

    00.20.40.60.81Intensity (arb. units)

    Rel

    ativ

    e en

    ergy

    (eV

    )FWHM= 1.3 eV

    Acceptance by Si 111 DCM

    Undulator radiation

  • 42

    Improvement of energy resolution

    (A) Collimation using slit (B) Collimation using pre-opticsw/ collimation mirror, CRL,..

    (C) Additional crystalw/ (+,+) setting

    (D) HR monochromator of π/2 reflection (~meV)

    Pho

    ton

    ener

    gy

    Angle

    ResolutionP

    hoto

    n en

    ergy

    Angle

    Resolution

    (B)~(D): restriction on photon energy

    Pho

    ton

    ener

    gy

    Angle

    Resolution

    Light source distribution

    Acceptance by crystal

    Pho

    ton

    ener

    gy

    Angle

    Resolution

    Slit width

  • 43

    Improvement of energy resolution(C) Additional crystal w/ (+,+) setting

    HXPES

    Si 111 DCM Si nnn channel-cut mono.

    Si 333 refl. for 6 keV

    Si 555 refl. for 10 keV

    40 μrad

    ΔE/E

    = 5x

    10-5

    -100

    -80

    -60

    -40

    -20

    0

    20

    40

    60

    80

    100

    00.20.40.60.81

    Intensity (arb. units)

    Rel

    ativ

    e en

    ergy

    (meV

    )

    -100

    -80

    -60

    -40

    -20

    0

    20

    40

    60

    80

    100

    00.20.40.60.81

    Intensity (arb. units)

    Rel

    ativ

    e en

    ergy

    (meV

    )

    FWHM= 45 meV

    FWHM= 18 meV

    Phot

    on e

    nerg

    y

    Angle

    Resolution

  • 44

    Improvement of energy resolution

    Si 111 DCM Si nnn back-scattering mono.

    Si 999 refl. for 17.8 keV

    Si 11 11 11 refl. for 21.7 keV

    20 μrad

    ΔE/E

    = 5x

    10-7

    (D) HR monochromator of ~π/2 reflection (~meV) Inelastic scattering

    Phot

    on e

    nerg

    y

    Angle

    Resolution

    -4

    -3

    -2

    -1

    0

    1

    2

    3

    4

    00.20.40.60.81

    Intensity (arb. units)

    Rel

    ativ

    e en

    ergy

    (meV

    )

    -4

    -3

    -2

    -1

    0

    1

    2

    3

    4

    00.20.40.60.81Intensity (arb. units)

    Rel

    ativ

    e en

    ergy

    (meV

    )

    FWHM= 2.0 meV

    FWHM= 0.87 meV

  • 45

    Photon flux after monochromatorPhoton flux (throughput) after monochromator can be estimated using effective band width:Photon flux (ph/s) =

    Photon flux from light source (ph/s/0.1%bw)

    x 1000

    x Effective band width of monochromator

    Throughput is estimated by overlapped area.

    Note difference from energy resolution.

    Pho

    ton

    ener

    gy Light source

    distribution

    Angle

    Effective band width

    Acceptance by crystal

  • 46

    Effective band width

    ( ){ }λλχ fdf hklhr ′+∝ )(02

    Independent of photon energy

    Starting with Darwin width in the energy axis

    )(02 hklhkl dfdEE

    ∝Δ

    −=Δ

    λλ

    0

    0.2

    0.4

    0.6

    0.8

    1

    -5 -4 -3 -2 -1 0 1 2 3 4 5

    10 keV30 keV

    Ref

    lect

    ivity

    2(x10-4)

    1.4x10-4

    ΔE/E

    e.g. for Si 111 refl. DCM caseNote relative energy width is constant.

    B2sin θ

    χhrEE

    ≈Δ

    Neglecting anomalous scattering factor f’

    )(02 hklhr dfλχ ∝

    22

    B2

    4

    sin

    λχ

    θχ

    λλ

    hrhkl

    hr

    d

    EE

    =

    ≈Δ

    −=Δ

  • 47

    Effective band width (Integrated intensity)

    ∫=Δ dWWREE hr 2

    B2 )(sin2 θ

    χ

    0

    2

    4

    6

    8

    10

    12

    14

    0 20 40 60 80 100Photon energy (keV)

    Effe

    ctiv

    e ba

    nd w

    idth

    Si 111 refl.

    Si 311 refl.

    Si 511 refl., Si 333 refl.

    (x10-5)

    For double-crystal monochromator

    When you need flux Lower order (Si 111 refl.,..)

    When you need resolution Higher order (Si 311, Si 511 refl,..)

    Effective band-width is obtained

    by integration of reflection curve.

    = ~2

  • 48

    Photon flux at undulator beamline

    We can obtain photon flux of 1013~1014 ph/s/100 mA/mm2 using standard undulator sources and Si 111 reflections at SPring-8 beamlines.

    1010

    1011

    1012

    1013

    1014

    1015

    1016

    0 10 20 30 40 50Photon energy (keV)

    Pho

    ton

    flux

    (ph/

    s/10

    0 m

    A) (a) total flux

    (c)

    (d)

    (b) partial flux

    (a) Total flux @ 0.1% b.w.(b) After frontend slit

    1×1 mm2 @30 m(c) Si 111 refl. @10 keV

    Effective b.w. = 1.3x10-4(d) 3rd harmonics @30 keV

    Effective b.w. = 8.0x10-6

    Higher harmonics elimination more mirror or detuning of DCM

  • 49

    Double-crystal monochromator

    Fixed-exit operation for usability at experimental station.

    Choose suitable mechanism for energy range(Bragg angle range).

    Precision, stability, rigidity,...

    Offset h

    y θB

    O

    A B

    z

    1st crystal

    2nd crystal

    θBθB

    Exit beam B

    hyθsin2

    AB ==

    B

    hzθcos2

    OB ==

    Fixed-exit operation using rotation (θ) + two translation mechanism

  • 5050

    e.g. Double-crystal monochromator

    θ-stage

    Translation stage

    1st crystal

    2nd crystal

    θ-stage

    y

    h

    SPring-8 BL15XU

    KEK-PF BL-4CMatsushita et al., NIM A246 (1986)

    θ stage

    1st crystal2nd crystal

    θ rotation centerY1 stage

    Z-cam stage

    SPring-8 std. DCMYabashi et al., Proc. SPIE 3773, 2 (1999)

    θ1 + translation + θ2 computer link

    θ + two translation (2 cams)

    θ + two translation (1 cam)

    h= 25 mm, θB= 5~70°Offset h= 30 mm

    θB =3~27º for higher energy range

    h= 100 mm,

    θB= 5.7~72°(for lower energy range)

  • 51

    Crystal cooling

    熱伝達

    Qin T1

    T0

    Radiation & convection

    Heat conduction in crystalHeat transfer

    to coolant/holder Coolant/holder

    Crystal

    Why crystal cooling?Qin (Heat load by SR) = Qout (Cooling + Radiation,..)

    with temperature rise ΔTαΔT = Δd (d-spacing change)

    α: thermal expansion coefficientor Δθ (bump of lattice due to heat load)

    Miss-matching between 1st and 2nd crystals occurs: Thermal drift, loss of intensity, broadening of beam, loss of brightnessMelting or limit of thermal strain Broken !

    Solutions:(S-1) κ/α Larger(S-2) Contact area between crystal and coolant/holder

    larger(S-3) Irradiation area Larger,

    and power density smaller

    Figure of meritSilicon Silicon Diamond300 K 80 K 300 K

    κ (W/m/K) 150 1000 2000α (1/K) 2.5x10-6 -5x10-7 1x10-6

    κ/α x106 60 2000 2000

    We must consider:- Thermal expansion of crystal: α,- Thermal conductivity in crystal: κ,- Heat transfer to coolant and crystal holder.

    Figure of merit of cooling:Good for silicon (80 k)

    and diamond (300 K)

  • 52

    Crystal cooling at SPring-8

    Linear undulator, N= 140, λu= 32 mm

    Power & power density: 300~500 W , 300~500 W/mm2

    a) Direct cooling of silicon pin-postcrystal – (S2) & (S3)

    b) Silicon cryogenic cooling - (S1)

    c) IIa diamond with indirect water cooling - (S1)

    0.6 mm

    0.6 mm

    0.5 mm

    0.2 mm

    Water flow

    Water flow

    X-rays

    O-ring

    Si-Au-Si bonding

    Power & power density:

    ~100 W, ~1 W/mm2

    Fin crystal direct-cooling - (S2)

  • 53

    Example of x-ray beamline- SPring-8 case -

  • 54

    XAFS & single crystal diffraction

    - Bending magnet- Collimator mirror, + DCM,+ refocusing mirror

    Roller

    ShaftLink

    Motor

    (a)

    (b)

    Bellows

    x

    Beamline center

    Collimatormirror

    Double-crystalmonochromator

    Gammastopper

    Downstreamshutter

    G1-G3: Gear box

    Refocusingmirror

    J1-J6: Jack

    Fixed point

    Ideal reflection axis

    (0, h)

    (x0, y0)h-y0

    J1 J2 J3 J4 J5 J6G1 G2 G3

  • 5555

    Protein crystallography

    - Bending magnet- DCM + focusing mirror

    Focusing mirror(Vertical deflection)

    Double-crystalmonochromator

    Shielded tube

    Optics hutch with standard components

    Experimental hutch

    Distance from the source50 m30 m 40 m

  • 56

    High resolution inelastic scattering- Undulator- DCM + back-reflection monochromator & analyzer (w/ ~meV resolution)

    Double-crystalmonochromator

    Downstream shutter 1

    Dual movableend-stopper

    Experimental hutch 3(Back scattering hutch)

    Experimental hutch 4(Analyzer hutch)

    Experimentalhutch 2

    Experimentalhutch 1

    Optics hutch

    Downstream shutter 2(Dual shutter)

    Si 111 double-crystal beam displacerFocusing mirror

    Downstream shutter 3 Back scattering

    monochromator

    Shielded beam ductSample position

    Inclination stage

    Distance from the source60 m30 m 40 m 50 m 70 m 80 m

    5

  • 57

    200-m-long beamline

    - Bending magnet- DCM

    Biomedical imaging centerExperimental hutch 2 and 3

    Distance from the source220 m200 m180 m160 m140 m120 m

    120 m100 m80 m60 m40 m

    Dry pump

    Dry pump

    Beam monitor andgate valve

    Roots pump with dry pump

    Arcade400-mm-diameter shielded beam duct

    Front end

    Experimental hutch 1

    Storage ring building

    Optics hutch with standard transport channel and optics

    300-mm-wide beam at end-station

  • 58

    SummaryKey issues on the x-ray monochromator were shown,

    introducing the dynamical x-ray diffraction for large & perfect crystal,

    w/ several important points:

    1) Total reflection occurs at the gap between dispersion surfaces.

    2) Normalized deviation parameter W is related to the gap.

    3) W is parameter of angular deviation and energy (wavelength) deviation.

    It gives DuMond diagram as a band of |W|

  • 59

    Text books following Laue’s dynamical theory

    Ergebnisse der Exakt Naturwiss.

    10 (1931) 133-158.

    R. W. James

    “The Dynamical Theory of X-Ray Diffraction”

    Solod State Physics 15, (1963) 53-220.

    Dover (1945)

    Oxford (2001)

    B. W. Batterman & H. Cole

    “Dynamical Diffraction of X-Rays by Perfect Crystals”

    Rev. Modern Phys. 36,

    (1964) 681-717.Springer (2004)

  • 60

    References

    For monochromator[1] T. Matsushita & H. Hashizume,

    Handbook on Synchrotron Radiation Vol. 1,

    North-Holland (1983).

    [2] Y. Shvyd’ko, Springer (2004), for high energy resolution

    For atomic scattering factorFor f0

    [3] International Tables for X-ray Crystallography (IUCr).[4] Hubbell et al.: J. Phys. Chem. Ref. Data Vol. 4, No. 3, 1975.For anomalous scattering factor f’, f”

    [5] S. Sasaki, KEK report 88-14 (1989),[6] Tables of LBNL (B. L. Henke et al.),

    http://henke.lbl.gov/optical_constants/index.html,[7] Tables of NIST,

    http://physics.nist.gov/PhysRefData/FFast/html/form.htm

  • 61

    Thanks to:

    H. Kitamura, T. Tanaka, S. Takahashi, K. Takeshita,

    N. Nariyama, Y. Asano, H. Ohashi, T. Mochizuki,

    M. Yabashi, H. Yamazaki, K. Tamasaku, A. Baron,

    M. Suzuki, T. Uruga, T. Matsushita, T. Ohata,

    Y. Furukawa, and T. Ishikawa

  • 62

    Thank you for your attention.